DOC PREVIEW
UA PTYS 554 - Lecture Notes

This preview shows page 1-2-3-27-28-29 out of 29 pages.

Save
View full document
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience
Premium Document
Do you want full access? Go Premium and unlock all 29 pages.
Access to all documents
Download any document
Ad free experience

Unformatted text preview:

PowerPoint PresentationSlide 2Slide 3Slide 4Slide 5Slide 6Slide 7Slide 8Slide 9Slide 10Late Southern Fall (Ls = 86˚, 2 PM)Slide 12Slide 13Slide 14Slide 15Slide 16Slide 17Slide 18Slide 19Slide 20Slide 21Slide 22Slide 23Slide 24Slide 25Slide 26Slide 27Slide 28Slide 29PTYS 554Evolution of Planetary SurfacesAeolian Processes IIAeolian Processes IIPYTS 554 – Aeolian Processes II2Aeolian Processes IEntrainment of particles – settling timescalesThreshold friction speedsSuspension vs. saltation vs. reptation vs. creepDependences on gravity, densities of particle/airAeolian Processes IIMigration ratesDune typesDunefield pattern formationRipples vs. dunesVentifact, yardang erosionDust-devils and wind streaksPYTS 554 – Aeolian Processes II3Reminders from last lecture…Surface shear stress from the wind is often expressed as a shear velocity:Law of the wall predicts logarithmic wind velocity (u) changes with height (z):Where z0 is a surface roughness length scaleBalancing particle weight and wind shear stress we can calculate (with an empirical constant, A) the threshold shear stress or velocity:A2 more commonly called θ in fluvial studiesA also a function of fluid:particle density ratio ‘A’ is a function of Reynolds number so that very small particles (hiding in the laminar sub-layer) are harder to mobilize than larger particles.A preferred particle size exists that is sand-sized u*=tra uu*=1klnzzoæ è ç ö ø ÷ tT=A2rs- ra( )gdéëùû u*T=Ars- raraæ è ç ö ø ÷ gdPYTS 554 – Aeolian Processes II4One core expression for mass flux (q)There are many variations fit to empirical dataGreeley, 1985q»ragu*3PYTS 554 – Aeolian Processes II5Sand tends to stick in sandy areas and bounce quickly across rocky surfacesLow hills of sand feel asymmetric shear stressTurbulent shear stress at many wavelengths combined linearlyJackson and Hunt 1975Doesn’t work so well when slopes > 10-15°Shear stress drops to zero when slopes exceed ~ 25° (back-pressure effects)Pelletier 2009PYTS 554 – Aeolian Processes II6Formation of a dune…Asymmetric shear stress causes lee-slope of all low hills to steepen Lee slopes steepen past 25°Air flow separates from lee-slope surfaceSand falls onto the upper lee-slope and is not removed causing steepeningLee slope approaches angle of reposeSlope controlled by gain avalanchesDune advancesStossSlopeNegative mass balanceLeeSlopePositive mass balanceFlatNeutral mass balance qµ u*3µ t32PYTS 554 – Aeolian Processes II7Dune velocityMass sand flux: qSome fraction (f) of this comes from the dune itselfDune Velocity:Bigger dunes move slower for a given sand fluxDunefields with similar sized dunes are stableDune height is self-limiting due to streamline compressionhDxDt=2 f qrduneæèçöø÷h- 1PYTS 554 – Aeolian Processes II8Upwind: Stoss sideDownwind: Lee sideHighest point: crestSlipface start: BrinkDunesStossLeeHornHornPYTS 554 – Aeolian Processes II9Unidirectional windsDune shape depends on sand supplyBarchan Barchanoid ridges TransverseIncreasing sand supplyPYTS 554 – Aeolian Processes II10Barchan dunes provide valuable wind direction measurementsPYTS 554 – Aeolian Processes II11Late Southern Fall (Ls = 86˚, 2 PM)Late Southern spring (Ls = 286˚, 4 PM)Surface geology can be tied to atmospheric modelingIndicates the dunes formed under current wind directionsLate Southern spring (Ls = 286˚, 4 PM)Fenton et al.PYTS 554 – Aeolian Processes II12When wind directions varyLinear dunes – a little variationStar dunes – a lot of variationStar Linear/LongitudinalPYTS 554 – Aeolian Processes II13Longitudinal dunes on TitanLorenz et al., 2006PYTS 554 – Aeolian Processes II14Titan’s dunes cover a significant portion of the bodyWinds blow from west to east… opposite to what models predictRadibaugh & LorenzPYTS 554 – Aeolian Processes II15For fast dune (large disparity in dune size) collisions…A perturbation to a dune size leads to runaway growthDune interactions and dunefieldsPYTS 554 – Aeolian Processes II16CollisionsDunes have a separation bubble(zone of zero shear stress)Allows upwind dune to take sand from the downwind duneDune-size ratio close to 1Interaction is slowUpwind dune steals sand until size ratio is reversedDownwind dune is now faster and escapesDune-size ratio far from 1Interaction is fastDunes mergeDiniega et al. 2010PYTS 554 – Aeolian Processes II17Dune field pattern formationA stable dune field has dunes all roughly the same sizeConsider Incoming size ratio vs. Outgoing size ratio in collisionsOutgoing size ratio > IncomingDunes are closer to equal sizedNext collision will make the size ratios even closer to oneEquilibrium reached when all the dunes are the same size (also means no more collisions)Outgoing size ratio < IncomingDunes are more different in size after a collisionIf size ratio is too small then collisions get too fast and mergers start happeningOutgoing size ratio = IncomingSoliton-like behavior (misleading analogy) where dunes appear to pass through each otherDuran et al. 2005Herrmann et al. 2005PYTS 554 – Aeolian Processes II18Form perpendicular to wind directionMuch more dynamic than dunesAsymmetric, 8-10 vs 20-30 degree slopesSeparation bubbles, but not slip facesWavelengths 0.5cm to 25m (mega-ripples)Typical wavelengths 7-14cm, heights 0.5-1cmRipple index: L / Height, typically ~18Wavelength related to grain-size(but also wind speed…)RipplescmDL75.08.63Pelletier 2009PYTS 554 – Aeolian Processes II19Bagnold again…Saltation path length ~ wavelengthHigh angle impacts erode material from Stoss sideLow angle impacts deposit material in shadow zoneCoarse-grained material tends to get concentrated on the crestsPYTS 554 – Aeolian Processes II20YardangsWind blown particles abrades surfaceErosion leaves elongated mounds as remnantsRequires strong, virtually unidirectional, wind.Eroded material must be consolidatedVentifactsElongated erosional marks on rocksUsually works on originally circular vesiclesUsed as paleo-wind direction indicators e.g. pathfinder landing siteAeolian ErosionOlder wind actionRecentwind actionPYTS 554 – Aeolian Processes


View Full Document
Download Lecture Notes
Our administrator received your request to download this document. We will send you the file to your email shortly.
Loading Unlocking...
Login

Join to view Lecture Notes and access 3M+ class-specific study document.

or
We will never post anything without your permission.
Don't have an account?
Sign Up

Join to view Lecture Notes 2 2 and access 3M+ class-specific study document.

or

By creating an account you agree to our Privacy Policy and Terms Of Use

Already a member?